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The Contact Binary H235 in the Open Cluster NGC 752

Published online by Cambridge University Press:  07 August 2017

E. F. Milone ,
C. R. Stagg ,
B.J.A. Sugars ,
J.R. Mcvean ,
S. J. Schiller  and
J. Kallrath
E. F. Milone
Affiliation:
RAO, Department of Physics and Astronomy, The University of Calgary, 2500 University Dr., NW, Calgary, Alberta, Canada T2N 1N4
C. R. Stagg
Affiliation:
RAO, Department of Physics and Astronomy, The University of Calgary, 2500 University Dr., NW, Calgary, Alberta, Canada T2N 1N4
B.J.A. Sugars
Affiliation:
RAO, Department of Physics and Astronomy, The University of Calgary, 2500 University Dr., NW, Calgary, Alberta, Canada T2N 1N4
J.R. Mcvean
Affiliation:
RAO, Department of Physics and Astronomy, The University of Calgary, 2500 University Dr., NW, Calgary, Alberta, Canada T2N 1N4
S. J. Schiller
Affiliation:
South Dakota State University, Department of Physics, Box 2219, Brookings, South Dakota 57007-0395
J. Kallrath
Affiliation:
Astronomische Institute der Universität Bonn and BASF-AG, D-7600 Ludwigshafen 1, Germany

Abstract

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Photoelectric BVRI light and radial velocity curves of the 0.41d period eclipsing variable have been analyzed with a new, simplex-enhanced version of the Wilson-Devinney light curve program, and used to explore detached, semi-detached, and contact solutions. The system is best modeled as a W-type W UMa system, with contact parameter, f = 0.44, although at time of writing, we cannot rule out the possibility of an A-type system.

Type
Oral and Contributed Papers
Information
Symposium - International Astronomical Union , Volume 151: Evolutionary Processes in Interacting Binary Stars , 1992 , pp. 487 - 490
Copyright
Copyright © Kluwer 1992 

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